Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Hicks, EKS"'
Publikováno v:
The Astrophysical Journal, vol 858, iss 1
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::d4c36c78795e14ec49247d31481d246f
https://escholarship.org/uc/item/2c064847
https://escholarship.org/uc/item/2c064847
Autor:
Davies, RI, Maciejewski, W, Hicks, EKS, Emsellem, E, Erwin, P, Burtscher, L, Dumas, G, Lin, M, Malkan, MA, Mueller-Sanchez, F, Xivry, GOD, Rosario, DJ, Schnorr-Mueller, A, Tran, A
Publikováno v:
Davies, RI; Maciejewski, W; Hicks, EKS; Emsellem, E; Erwin, P; Burtscher, L; et al.(2017). Fueling AGN II: Spatially Resolved Molecular Inflows and Outflows. UCLA: Retrieved from: http://www.escholarship.org/uc/item/6fb7d6cr
We analyse the 2-dimensional distribution and kinematics of the stars as well as molecular and ionised gas in the central few hundred parsecs of 5 active and 5 matched inactive galaxies. The equivalent widths of the Br-gamma line indicate there is no
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1ff4b1154d418c8174a0be4fcb560ec5
Autor:
Hicks, EKS, Davies, RI, Maciejewski, W, Emsellem, E, Malkan, MA, Dumas, G, Müller-Sánchez, F, Rivers, A
Publikováno v:
The Astrophysical Journal, vol 768, iss 2
In a matched sample of Seyfert and quiescent galaxies we simultaneously probe the stellar and molecular gas kinematics from 1 kpc down to 50 pc with the aim of identifying the dynamical processes dictating black hole accretion rates. This first paper
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::3c79f26fb9ba9b990280cd7862a6eb93
https://escholarship.org/uc/item/4f06z7qp
https://escholarship.org/uc/item/4f06z7qp
Autor:
Schreiber, NMF, Genzel, R, Bouche, N, Cresci, G, Davies, R, Buschkamp, P, Shapiro, K, Tacconi, LJ, Hicks, EKS, Genel, S, Shapley, AE, Erb, DK, Steidel, CC, Lutz, D, Eisenhauer, F, Gillessen, S, Sternberg, A, Renzini, A, Cimatti, A, Daddi, E, Kurk, J, Lilly, S, Kong, X, Lehnert, MD, Nesvadba, N, Verma, A, McCracken, H, Arimoto, N, Mignoli, M, Onodera, M
Publikováno v:
ASTROPHYSICAL JOURNAL. 706(2)
We present the Spectroscopic Imaging survey in the near-infrared (near-IR) with SINFONI (SINS) of high-redshift galaxies. With 80 objects observed and 63 detected in at least one rest-frame optical nebular emission line, mainly Hα, SINS represents t
Publikováno v:
The Astrophysical Journal, vol 696, iss 1
In a sample of local active galactic nuclei (AGNs) studied at a spatial resolution on the order of 10 pc, we show that the interstellar medium traced by the molecular hydrogen ν = 1-0 S(1) line at 2.1 μm forms a geometrically thick, clumpy disk. Th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______325::d3c7f7d51bd5ae48b3b537bd18947a30
https://escholarship.org/uc/item/4cv0r5sw
https://escholarship.org/uc/item/4cv0r5sw
Autor:
Hicks, EKS, Malkan, MA
Publikováno v:
Hicks, EKS; & Malkan, MA. (2008). Circumnuclear gas in seyfert 1 galaxies: Morphology, kinematics, and direct measurement of black hole masses. Astrophysical Journal, Supplement Series, 174(1), 31-73. doi: 10.1086/521650. UCLA: Retrieved from: http://www.escholarship.org/uc/item/9640c57x
Astrophysical Journal, Supplement Series, vol 174, iss 1
Astrophysical Journal, Supplement Series, vol 174, iss 1
The two-dimensional (2D) distribution and kinematics of the molecular, ionized, and highly ionized gas in the nuclear regions of Seyfert 1 galaxies have been measured using high spatial resolution (∼0.09'') near-infrared spectroscopy from NIRSPEC w
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::267d6987601f60aace825322d59b21aa
http://www.escholarship.org/uc/item/9640c57x
http://www.escholarship.org/uc/item/9640c57x
Akademický článek
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Autor:
Caglar, T, Burtscher, L, Brandl, B, Brinchmann, J, Davies, R, Hicks, EKS, Koss, M, Lin, M-Y, Maciejewski, W, Mueller-Sanchez, F, Riffel, RA, Riffel, R, Rosario, DJ, Schartmann, M, Schnorr-Mueller, A, Shimizu, TT, Storchi-Bergmann, T, Veilleux, S, de Xivry, GO, Bennert, VN
Context. The MBH–σ⋆ relation is considered a result of coevolution between the host galaxies and their supermassive black holes. For elliptical bulge hosting inactive galaxies, this relation is well established, but there is still discussion con
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=core_ac_uk__::3315c551d5386cb304cb954dca736ed8
https://researchonline.ljmu.ac.uk/id/eprint/12687/1/aa36321-19.pdf
https://researchonline.ljmu.ac.uk/id/eprint/12687/1/aa36321-19.pdf